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  • 1
    Publication Date: 2011-12-07
    Description: Author(s): L. X. Han (韩立欣), G. L. Ma (马国亮), Y. G. Ma (马余刚), X. Z. Cai (蔡翔舟), J. H. Chen (陈金辉), S. Zhang (张松), and C. Zhong (钟晨) [Phys. Rev. C 84, 064907] Published Tue Dec 06, 2011
    Keywords: Relativistic Nuclear Collisions
    Print ISSN: 0556-2813
    Electronic ISSN: 1089-490X
    Topics: Physics
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  • 2
    Publication Date: 2011-04-19
    Description: Author(s): L. X. Han (韩立欣), G. L. Ma (马国亮), Y. G. Ma (马余刚), X. Z. Cai (蔡翔舟), J. H. Chen (陈金辉), S. Zhang (张松), and C. Zhong (钟晨) A potential experimental probe, the forward-backward elliptic anisotropy correlation (C_{FB} ), has been proposed by Liao and Koch to distinguish the jet and true elliptic flow contribution to the measured elliptic flow (v_{2} ) in relativistic heavy-ion collisions. The jet and flow fluctuation cont... [Phys. Rev. C 83, 047901] Published Mon Apr 18, 2011
    Keywords: Relativistic Nuclear Collisions
    Print ISSN: 0556-2813
    Electronic ISSN: 1089-490X
    Topics: Physics
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  • 3
    Publication Date: 2014-04-01
    Description: Author(s): S. Zhang (张松), L. X. Han (韩立欣), Y. G. Ma (马余刚), J. H. Chen (陈金辉), and C. Zhong (钟晨) The particle production and their ratios for π, K, p, and Λ are studied in Pb + Pb collisions at sNN=2.76 TeV based on a blast-wave model with thermal equilibrium mechanism. The transverse momentum spectra of the above-mentioned particles at the kinetic freeze-out stage are discussed. The modificati... [Phys. Rev. C 89, 034918] Published Mon Mar 31, 2014
    Keywords: Relativistic Nuclear Collisions
    Print ISSN: 0556-2813
    Electronic ISSN: 1089-490X
    Topics: Physics
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  • 4
    Publication Date: 2010-01-08
    Description: The ability to silence the activity of genetically specified neurons in a temporally precise fashion would provide the opportunity to investigate the causal role of specific cell classes in neural computations, behaviours and pathologies. Here we show that members of the class of light-driven outward proton pumps can mediate powerful, safe, multiple-colour silencing of neural activity. The gene archaerhodopsin-3 (Arch) from Halorubrum sodomense enables near-100% silencing of neurons in the awake brain when virally expressed in the mouse cortex and illuminated with yellow light. Arch mediates currents of several hundred picoamps at low light powers, and supports neural silencing currents approaching 900 pA at light powers easily achievable in vivo. Furthermore, Arch spontaneously recovers from light-dependent inactivation, unlike light-driven chloride pumps that enter long-lasting inactive states in response to light. These properties of Arch are appropriate to mediate the optical silencing of significant brain volumes over behaviourally relevant timescales. Arch function in neurons is well tolerated because pH excursions created by Arch illumination are minimized by self-limiting mechanisms to levels comparable to those mediated by channelrhodopsins or natural spike firing. To highlight how proton pump ecological and genomic diversity may support new innovation, we show that the blue-green light-drivable proton pump from the fungus Leptosphaeria maculans (Mac) can, when expressed in neurons, enable neural silencing by blue light, thus enabling alongside other developed reagents the potential for independent silencing of two neural populations by blue versus red light. Light-driven proton pumps thus represent a high-performance and extremely versatile class of 'optogenetic' voltage and ion modulator, which will broadly enable new neuroscientific, biological, neurological and psychiatric investigations.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2939492/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2939492/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Chow, Brian Y -- Han, Xue -- Dobry, Allison S -- Qian, Xiaofeng -- Chuong, Amy S -- Li, Mingjie -- Henninger, Michael A -- Belfort, Gabriel M -- Lin, Yingxi -- Monahan, Patrick E -- Boyden, Edward S -- 1K99MH085944/MH/NIMH NIH HHS/ -- DP2 OD002002/OD/NIH HHS/ -- DP2 OD002002-01/OD/NIH HHS/ -- K99 MH085944/MH/NIMH NIH HHS/ -- K99 MH085944-01/MH/NIMH NIH HHS/ -- England -- Nature. 2010 Jan 7;463(7277):98-102. doi: 10.1038/nature08652.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉The MIT Media Laboratory, Synthetic Neurobiology Group, and Department of Biological Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20054397" target="_blank"〉PubMed〈/a〉
    Keywords: Action Potentials/radiation effects ; Animals ; Ascomycota/metabolism/radiation effects ; Color ; Electric Conductivity ; Euryarchaeota/metabolism/radiation effects ; Genetic Engineering/*methods ; Hydrogen-Ion Concentration ; Mice ; Molecular Sequence Data ; Neocortex/cytology/physiology/radiation effects ; Neurons/*metabolism/*radiation effects ; Proton Pumps/classification/genetics/*metabolism/*radiation effects ; Rhodopsins, Microbial/antagonists & inhibitors/genetics/metabolism/radiation ; effects ; Wakefulness
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 5
    Publication Date: 2013-01-12
    Description: An extensive literature shows that astrocytes exhibit metabotropic glutamate receptor 5 (mGluR5)-dependent increases in cytosolic calcium ions (Ca(2+)) in response to glutamatergic transmission and, in turn, modulate neuronal activity by their Ca(2+)-dependent release of gliotransmitters. These findings, based on studies of young rodents, have led to the concept of the tripartite synapse, in which astrocytes actively participate in neurotransmission. Using genomic analysis, immunoelectron microscopy, and two-photon microscopy of astrocytic Ca(2+) signaling in vivo, we found that astrocytic expression of mGluR5 is developmentally regulated and is undetectable after postnatal week 3. In contrast, mGluR3, whose activation inhibits adenylate cyclase but not calcium signaling, was expressed in astrocytes at all developmental stages. Neuroglial signaling in the adult brain may therefore occur in a manner fundamentally distinct from that exhibited during development.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3569008/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC3569008/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Sun, Wei -- McConnell, Evan -- Pare, Jean-Francois -- Xu, Qiwu -- Chen, Michael -- Peng, Weiguo -- Lovatt, Ditte -- Han, Xiaoning -- Smith, Yoland -- Nedergaard, Maiken -- NS075177/NS/NINDS NIH HHS/ -- NS078304/NS/NINDS NIH HHS/ -- P51OD011132/OD/NIH HHS/ -- P51RR000165/RR/NCRR NIH HHS/ -- R01 NS075177/NS/NINDS NIH HHS/ -- R01 NS078167/NS/NINDS NIH HHS/ -- R01 NS078304/NS/NINDS NIH HHS/ -- RR00165/RR/NCRR NIH HHS/ -- New York, N.Y. -- Science. 2013 Jan 11;339(6116):197-200. doi: 10.1126/science.1226740.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Division of Glial Disease and Therapeutics, Center for Translational Neuromedicine, University of Rochester, Rochester, NY 14642, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23307741" target="_blank"〉PubMed〈/a〉
    Keywords: Adolescent ; *Aging ; Animals ; Astrocytes/*metabolism ; Calcium/metabolism ; *Calcium Signaling ; Cerebral Cortex/cytology/*metabolism/ultrastructure ; Female ; Glutamic Acid/*metabolism ; Hippocampus/cytology/metabolism/ultrastructure ; Humans ; Male ; Mice ; Mice, Inbred C57BL ; Receptor, Metabotropic Glutamate 5 ; Receptors, Metabotropic Glutamate/agonists/*metabolism ; Synaptic Transmission
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 6
    Publication Date: 2019-07-13
    Description: We have monitored the evolution of the transient X-ray source GRO J0422+32 from approximately 2 weeks postdiscovery into its early decline phase at ultraviolet, optical, and radio wavelengths. Optical and ultraviolet spectra exhibit numerous, but relatively weak, high-excitation emission lines such as those arising from He II, N III, N V, and C IV superposed on an intrinsically blue continuum. High-resolution optical spectroscopy reveals line profiles which are double peaked, and in the case of the higher order Balmer lines, superposed on a broad absorption profile. The early outburst optical-ultraviolet continuum energy distribution is well represented by a two power-law fit with a break at approximately equal 4000 A. Radio observations with the Very Large Array (VLA) reveal a flat-spectrum source, slowly increasing in intensity at the earliest epochs observed, followed by an approximate power-law decay light curve with an index of -1. Light curves for each wavelength domain are presented and discussed. Notable are the multiple secondary outbursts seen in the optical more than 1 year postdiscovery, and spectral changes associated with secondary rises seen in the radio and UV. We find that the ultraviolet and optical characteristics of GRO J0422+32 as well as its radio evolution, are similar to other recent well-observed soft X-ray transients (also called X-ray novae) such as Cen X-4, A0620-00 (V616 Mon), and Nova Muscae 1991 (GS 1124-683), suggesting that GRO J0422+32 is also a member of that subclass of low-mass X-ray binaries. We present definitive astrometric determination of the source position, and place an upper limit of R approximately equals 20 from our analysis of the Palomar Observatory Sky Survey (POSS). Additionally, we derive distinct values for color excess from analysis of the optical (E(B-V) = 0.23) and ultraviolet (E(B-V) = 0.4) data, suggesting an intrinsic magnitude of 19-19.5 for the progenitor if it is mid-K dwarf. This leads to a likely range of 2.4-3.0 kpc for the source distance, which is consistent with our separate estimate of 2.4 +/- 0.4 kpc based on measurement of the NaD interstellar line profile. Adopting 2.4 kpc and E(B-V) = 0.23, the outburst absolute magnitude was M approximately equals 0.0, which is a typical value for this class of objects.
    Keywords: ASTRONOMY
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 434; 2; p. 698-706
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  • 7
    Publication Date: 2019-07-13
    Description: On May 22, 1989, the Japanese Ginga Team discovered a new x ray source that was cataloged as GS 2023+338. This source was subsequently identified as coincident in position with a previously known nova cataloged as V404 Cygni. Its last recorded outburst was in 1938 when it rose to about 12th mag. Spectroscopic data were obtained and confirmed the nature of the outburst. Additional ground based data were obtained by us at CTIO and the VLA. The x ray behavior of this object was reported to be very unusual and it reached a peak of about 17 crab about one week after discovery. Since then it has varied widely in magnitude at all wavelengths at which it has been studied. A brief summary of the observations that were obtained up to the time of the meeting and shortly thereafter is presented.
    Keywords: ASTRONOMY
    Type: DE90-008935 , LA-UR-90-875 , CONF-8906225-4 , IAU Coll. No. 122 on Physics of Classical Novae; Jun 27, 1989 - Jun 30, 1989; Madrid; Spain
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